Випущено: 2019 Feb 20 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
20 Feb 2019 | 070 | 010 |
21 Feb 2019 | 070 | 018 |
22 Feb 2019 | 070 | 008 |
Solar activity was at very low levels. An A9.7 flare peaked at 04:24 UT and was related to the eruption of the filament in former active region NOAA 2733 between 04 and 05 UT. This filament is reshaping itself and is currently located near N10E00. Associated with this eruption was a narrow and very slow moving (190 km/s) coronal mass ejection (CME) with a potential earth-directed component (STEREO-A/COR2 imagery). A preliminary estimate of the CME arrival near Earth is 26 February. The greater than 10 MeV proton flux was at nominal values.
Solar activity is expected to remain at very low levels.
Solar wind speed showed a generally declining trend from 340 km/s at the beginning of the period to 300 km/s at the end (DSCOVR). Bz ranged between -3 and +2 nT, with solar wind proton density gradually increasing to its current 10/cm3. The interplanetary magnetic field was mainly directed towards the Sun (negative sector). Geomagnetic activity was at quiet levels.
Mostly quiet geomagnetic conditions are expected until the arrival of the co-rotating interaction region and wind stream from the positive polarity coronal hole later today or on 21 February. This may result in active conditions, with a small chance on an isolated minor storming episode.
Today's estimated international sunspot number (ISN): 000, based on 19 stations.
Wolf number Catania | 012 |
10cm solar flux | 070 |
AK Chambon La Forêt | 005 |
AK Wingst | 003 |
Estimated Ap | 002 |
Estimated international sunspot number | 000 - Based on 28 stations |
Day | Begin | Max | Кінець | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
---|---|---|---|---|---|---|---|---|---|---|
Немає |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
Весь час у UTC
Багато людей відвідують сайт SpaceWeatherLive, щоб слідкувати за сонячною та авроральною активністю, але зі збільшенням трафіку хостинг також стає дорожчим. Будь-ласка, подумайте про пожертву, якщо вам подобається SpaceWeatherLive, щоб ми могли і надалі підтримувати цей сайт і платити за хостинг!
Останній X-спалах | 2025/03/28 | X1.1 |
Останній M-спалах | 2025/04/01 | M2.5 |
Останній геомагнітний шторм | 2025/03/27 | Kp5 (G1) |
Дні без сонячних плям | |
---|---|
Останній день без сонячних спалахів | 2022/06/08 |
Середня кількість сонячних плям протягом місяця | |
---|---|
лютого 2025 | 154.6 +17.6 |
квітня 2025 | 152.5 -2.1 |
Останні 30 днів | 130.7 -17.9 |